Influence of Mineral Composition of Melaphyre Grits on Durability of Motorway Surface

Total Page:16

File Type:pdf, Size:1020Kb

Influence of Mineral Composition of Melaphyre Grits on Durability of Motorway Surface Physicochemical Problems of Mineral Processing, 38 (2004) 341-350 Fizykochemiczne Problemy Mineralurgii, 38 (2004) 341-350 Tadeusz CHRZAN4 INFLUENCE OF MINERAL COMPOSITION OF MELAPHYRE GRITS ON DURABILITY OF MOTORWAY SURFACE Received April 4, 2004; reviewed; accepted June 5; 2004 The surface layer of the Konin-Września motorway section was made between July and November of 2001. Although the tests of melaphyre aggregates against grade and class requirements had confirmed that grits were the first class and grade according to the Polish standards, the motorway has been wearing rapidly with the first repairs being carried out as early as 2003. The motorway surface has been excessively worn and looks as if it were used for at least 5 years. The paper explains why the motorway surface has been worn so rapidly. Key words: motorway, ,melaphyre grit, weathering INTRODUCTION The surface layer of the Konin-Września motorway section was made during the period from July to November 2001. The layer was made with granulated aggregate 0- 20 mm in diameter from Borówko and Grzędy melaphyre quarry, bounded with modified bituminous mass. The tests of melaphyre aggregates against grade and class requirements had confirmed that the grits were the first class and grade (Chrzan, 1997; Wysokowski, 2000/2001) according to the Polish Standards (PN-11112:96, PN- 11110:96, PN-EN 1097-2). The binding layer of asphaltic concrete made and tested on samples that were taken from the completed motorway also conformed to the standard requirements according to Polish Standards (PN-S/96025, PN-74/S-96022). Also, the adhesion of asphalt to the melaphyre grit conformed to the standard (PN-84/B-6714/22). After the wintertime, in spring 2002, on the surface of the roadway, distinct signs of scaling and weathering were observed on the surface of larger melaphyre grit grains. In August 2002, it was found that the number of weathered grains had 4 Institute of Environmental Engineering, University of Zielona Góra, Poland 342 T. Chrzan increased and some of them lost their compactness and disintegrated (Ruttmar, 2002). Between September and November of 2003, due to the above reason, which threatened the safety of moving vehicles, partial repairs were carried out covering 1600 square metres. The surface of motorway has been excessively worn and looks as if it were used for at least 5 years. In this paper, it is explained why the motorway has been worn so quickly. ANALYSIS OF DECREASE OF ASPHALTIC CONCRETE STRENGTH OF MOTORWAY A2 BINDING LAYER IN RESPECT TO MINERAL COMPOSITION OF ROCKS DESCRIPTION OF MELAPHYRE DEPOSIT (Radziszewska-Jargosz, 1982; Szuszkiewicz I Król, 1988) The melaphyre used for road construction come from deposit that was formed from basalt-type volcanic rocks in the Permian period around 350 mln million years ago. The volcanic rocks created trachyte-basalt, trachyte and tuff-type rocks. The melaphyre deposit is exploited in the quarries of Borówno, Grzędy and Rybnica Leśna. The trachyte basalts are of two types. The first one includes rocks coloured cherry-brown, cherry-brick and grey-violet. They have chaotic structure and aphanitic texture. Cracks are filled with the ferruginous and carbonate substance. The second type is the rock ranging from grey-brown through grey-greenish to nearly black in colour. The structure is aphanitic and the texture is dense. Course- grained breccia of chaotic texture is also found. Volcanic spalls are cemented with the ferruginous and carbonate binder. The rock spalls are grey-brown and are of various size and aphanitic structure. The tuffs are cherry-brown, have aphanitic structure and chaotic, texture. They disintegrate into irregular small blocks. Numerous quartz grains and carbonate veins are visible. The sedimentary rocks are cherry-brown in colour and have fine-grained structure with directional texture. They disintegrate into irregular small blocks. Rocks of lava- mudstone fraction are found in the deposit which may have been the result of lava flooding during volcano eruption of weathered layers from the previous outflow. The exploited rock is melaphyre-type aphanite lava ranging from dark grey to black in colour; solid but intensely cracked rock. The cracks make it vulnerable to weathering and 0-10 mm sized rock is dumped as waste (Kancler, 2002a) in amount of 21% at Borówno quarry, and 15% at Grzędy quarry (Kancler, 2002b). This gives evidence that malaphyre in the Borówno quarry is built from minerals that are subject of stronger weathering than that in the Grzędy quarry. The melaphyre (Kancler, 2002a and 200b) in both quarries is built from minerals that disintegrate under the influence of temperature, air and water. Influence of mineral composition of melaphyre grits on durability of motorway surface 343 PETROGRAPHIC ANALYSIS OF MELAPHYRE The petrographic analysis of Grzędy deposit (Radziszewska-Jargosz, 1982) shows that plagioclases are found in the form of small phenocrysts. Feldspars undergo the process of sericitization and carbonization, and weathering processes lead to kaolinization. The ferruginous substance infiltrates the strips of plagioclases. Dark minerals were completely transformed. They were replaced with hydrated iron oxides accompanied by concentrations of carbonates, and in place of olivine there is a substance that is difficult to identify. Chlorite is rarely found. Pores are refilled with calcite accompanied by ferruginous pigment. In the pores there are concentrations of chalcedony. Concentrations of limonite are often found. Apatite, ilmenite and magnetite are accessory minerals. Volcanic glass, brown or orange in colour is also found. The rock groundmass consists of heavily carbonatizated glass, perches of plagioclases, ash fraction and iron oxides. PROPERTIES OF MINERALS FOUND IN THE MELAPHYRE DEPOSIT [Bolewski I Manecki, 1993; Bolewski, 1972; Chrzan, 1997) On the basis of geological documentation [8] on melaphyre deposit of the Borówno quarry, the mineralogical composition of fresh samples collected from the deposit is as follows: plagioclase 45.2-75.0 %, pyroxene 0-5.81 %, oxides and hydroxides 6.1-38.7 %, carbonates 0-8.3 %, chlorite 0-4.7 %, clayey minerals 0-5.2 %, quartz 0-3.0 %, iddingsite 0-9.7%, and unidentified 0-1.0 %. Feldspars (plagioclases) Plagioclases are sodium-calcium (Ca, Na) feldspars. Also found, there are potassium (K), white (Na) and lime (Ca) feldspars. The feldspars, more generally called aluminosilicates, form mixed crystals where K, Na, and Ca combined in different proportions among themselves and silica. Specific density of feldspars ranges from 2.5-2.8 Mg/m3. With an increase of calcium (Ca) content, plagioclases disintegrate easier into clay minerals, in particular into kaolinite. The kaolinization of plagioclases is commonly known among geologists. The weathering product of plagioclases that are rich in calcium is also calcite (CaCO3) coloured yellowish or brown. Kaolinite is the basic component of clayey minerals coloured red or brown and with specific density 2.5-2.6 Mg/m3, which is found in the form of dense or scaly concentrations. Wet kaolinite becomes plastic. The clayey minerals also include montmorillonite with specific density 2.0 Mg/m3 and in the form of white dense or scaly concentrations, which intensely swells in water, and decolourises denatured alcohol or methylene blue solution. Bentonite of the same colour and density behaves in a similar way; it is a mixture of clay minerals of the montmorillonite group. Feldspars also undergo the processes of sericitization and carbonisation. From the potassium feldspars, sericite is formed of scaly structure, and chlorite of scaly structure. 344 T. Chrzan Micas, such as muscovite, are found in the form of lamellas or lamella concentrations. These are minerals, formed of Na, K, Al, Fe, Mg, Si elements in various combinations. Mica is found in the magma rocks rich in SiO2 such as granites. In sedimentary rocks, it transforms into hydro-muscovite. They are green and black, yellow or brown in colour. Sericite has the form of tiny scales and is created at low hydrothermal temperatures. Sericitization takes place when feldspar turns to sericite. Pyroxenes Pyroxenes belong to aliphatic silicates and aluminosilicates. Group 1 consists of Mg-Fe, Mn-Mg, Ca, Ca-Na, Na-type pyroxenes. Pyroxenes is an important group of rock-forming minerals, which are created at high temperatures and at low water pressure. They are components of magma rocks and metamorphic rocks. They are not resistive to climatic factors, therefore are rarely found in sedimentary rocks. The colour of pyroxenes depends on iron and titanium content. At small content, it ranges from white to greenish, with larger content, it is olive, brown or dark green. Orthorhombic pyroxenes form the isomorphous series from Mg to Fe, with distinguished enstatite, bronzite, hypersthene, ferrohyperstene, eulite. Monoclinic pyroxenes include four minerals creating a diopsyde-hedenbergite series built from Ca, Mg, Fe, SiO2. Iron oxides and hydroxides Hematite (Fe2O3) has a cherry colour in variety of shades. It is insoluble. It may instantly oxidize in weak acids. In small quantities, it is found in magma rocks, especially those coloured red. It is a component of hydrothermal formations. Geothyte (FeOOH) ranges from brown to is red in colour. It is a product of hydrothermal activity at low temperature. It often occurs as an admixture colouring other rocks and in melaphyre vacuum. It is a product of iron mineral oxidation. Carbonates Calcite (CaCO3) is ranging from white to brown in colour. A component of sedimentary rocks, such as limestone, chalk, marls. It is formed in the hydrothermal activity zone independently fills rock crevices. Aragonite (CaCO3) is from white to brown in colour and is found in granular or dripstone crevices of melaphyres and basalts. It is a mineral of hydrothermal zone. Dolomite (CaMg(CO3)2) is a sedimentary rock mineral ranging from white to black in colour with density 2.8-2.9 Mg/m3 and is found in granular or dense form.
Recommended publications
  • Luís Pedro Esteves Internal Curing in Cement-Based Materials Universidade De Departamento De Engenharia Civil Aveiro 2009
    Universidade de Departamento de Engenharia Civil Aveiro 2009 Luís Pedro Esteves Internal curing in cement-based materials Universidade de Departamento de Engenharia Civil Aveiro 2009 Luís Pedro Esteves Internal curing in cement-based materials Dissertação apresentada à Universidade de Aveiro para cumprimento dos requisitos necessários à obtenção do grau de Doutor em Engenharia Civil, realizada sob a orientação científica do Dr. Paulo Barreto Cachim, Professor Associado do Departamento de Engenharia Civil da Universidade de Aveiro e do Dr. Victor Miguel C. de Sousa Ferreira, Professor Associado do Departamento de Engenharia Civil da Universidade de Aveiro. Beside other problematic, it was often astonishing to run after thoughts. As an ancient philosophy doctor pointed out: “The greater the attempt that is made to study the nature or behaviour of a photon or a particle, the greater will be the uncertainty or error of the measurements.” Heisenberg summarised this in his uncertainty principle, the concept being demonstrated by means of idealized “thought” experiments. If it is permitted for me to say, I would add: (…), provided that it can not be seen or felt. O júri PRESIDENTE: Reitora da Universidade de Aveiro VOGAIS: Doutor Ole Mejhede Jensen, Professor Catedrático da Technical University of Denmark. Doutor Klaas van Breugel, Professor Catedrático da Delft University of Technology. Doutor Aníbal Guimarães da Costa, Professor Catedrático da Universidade de Aveiro. Doutor José Luís Barroso de Aguiar, Professor Associado com Agregação da Universidade do Minho. Doutor Paulo Barreto Cachim, Professor Associado da Universidade de Aveiro (Orientador). Doutor Victor Miguel Carneiro de Sousa Ferreira, Professor Associado da Universidade de Aveiro (Co-Orientador).
    [Show full text]
  • Experimental Investigation of the Pressure of Crystallization of Ca(OH)2: Implications for the Reactive Cracking Process
    Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Experimental Investigation of the Pressure of Crystallization 10.1029/2018GC007609 of Ca(OH)2: Implications for the Reactive Cracking Process Key Points: S. Lambart1,2 , H. M. Savage1, B. G. Robinson1, and P. B. Kelemen1 • Crystallization pressure of CaO hydration exceeds 27 MPa at 1-km 1Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY, USA, 2Geology and Geophysics, University of Utah, crustal depth • Fluid transport via capillary flow is Salt Lake City, UT, USA rate limiting • Strain rate exhibits negative, power law dependence on uniaxial load Abstract Mineral hydration and carbonation can produce large solid volume increases, deviatoric stress, and fracture, which in turn can maintain or enhance permeability and reactive surface area. Supporting Information: Despite the potential importance of this process, our basic physical understanding of the conditions • Supporting Information S1 under which a given reaction will drive fracture (if at all) is relatively limited. Our hydration experiments • Table S2 on CaO under uniaxial loads of 0.1 to 27 MPa show that strain and strain rate are proportional to the • Table S3 square root of time and exhibit negative, power law dependence on uniaxial load, suggesting that (1) fl fl fi Correspondence to: uid transport via capillary ow is rate limiting and (2) decreasing strain rate with increasing con ning S. Lambart, pressure might be a limiting factor in reaction driven cracking at depth. However, our experiments also [email protected] demonstrate that crystallization pressure due to hydration exceeds 27 MPa (consistent with a maximum crystallization pressure of 153 MPa for the same reaction, Wolterbeek et al., https://doi.org/10.1007/ Citation: s11440-017-0533-5).
    [Show full text]
  • New Insights on the Prehydration of Cement and Its Mitigation 2 3 Julyan Stoian (I), Tandre Oey (Ii), Jeffrey W
    1 New Insights on the Prehydration of Cement and its Mitigation 2 3 Julyan Stoian (i), Tandre Oey (ii), Jeffrey W. Bullard (iii), Jian Huang (iv), Aditya Kumar (v), 4 Magdalena Balonis (vi,vii), Judith Terrill (viii), Narayanan Neithalath (ix), Gaurav Sant (x,xi) 5 6 Abstract 7 8 Ordinary portland cement (OPC) prehydrates during storage or handling in moist environments, 9 forming hydration products on or near its particles’ surfaces. Prehydration is known to reduce 10 OPC reactivity, but the extent of prehydration has not yet been quantitatively linked to reaction 11 rate and mechanical property changes. A series of experiments and simulations are performed 12 to develop a better understanding of prehydration, by intentionally exposing an OPC powder to 13 either water vapor or liquid water, to investigate the extent to which premature contact of OPC 14 with water and other potential reactants in the liquid and/or vapor state(s) can induce differing 15 surface modifications on the OPC grains. Original results obtained using isothermal calorimetry, 16 thermogravimetric analysis and strength measurements are correlated to a prehydration index, 17 which is defined for the first time. The addition of fine limestone to a mixture formed using 18 prehydrated cement is shown to mitigate the detrimental effects of prehydration. 19 20 Keywords: physisorption, prehydration, nucleation, limestone 21 22 23 1. Introduction and Background 24 Ordinary portland cement (OPC) reacts on contact with water in the liquid or the vapor states. 25 Therefore, unintentional exposure to moisture or to other known reactants such as CO2 during 26 the storage and handling of the OPC powder can result in premature hydrationxii or aging of its 27 constituent phases.
    [Show full text]
  • Performing Mineral Hydration Experiments in the Chemin Diffractometer on Mars
    Performing mineral hydration experiments in the CheMin diffractometer on Mars Session P009: Experimental Planetary Geochemistry: Simulating planetary processes on the Moon, Mars and other rocky bodies in the Solar System. D.T. Vaniman, A.S. Yen, E.B. Rampe, D.F. Blake, S.J. Chipera, J.M. Morookian, D.W. Ming, T.F. Bristow, R.V. Morris, R. Gellert, S.M. Morrison, J.P. Grotzinger, C.N. Achilles, R.T. Downs, W. Rapin, M. Rice, J.F. Bell III, A. H. Treiman, P. Sarrazin, and J.D. Farmer. Laboratory work is the cornerstone of experimental planetary geochemistry, mineralogy, and petrology, but much is to be gained by “experiments” while on a planet surface. Earth-bound experiments are often limited in ability to control multiple conditions relevant to planetary bodies (e.g. cycles in temperature and vapor pressure of water), but observations on-planet provide a unique opportunity where conditions are native to the planet and those affected by sampling and analysis can be constrained. The CheMin XRD instrument on Mars Science Laboratory has been able to test mineral hydration in samples held for up to 300 Mars days (sols). Clay minerals sampled at Yellowknife Bay early in the mission had both collapsed (10 Å) and expanded (13.2 Å) basal spacing. Collapsed interlayers were expected, but larger spacing was not; it was uncertain whether larger basal spacing would collapse on prolonged exposure to warmer conditions inside CheMin. Observation over several hundred sols showed no collapse, with the conclusion that expanded interlayer spacing was due to partial intercalation by metal-hydroxyl groups that resist dehydration.
    [Show full text]
  • Characterization of Hydrogen in Basaltic Materials with Laser-Induced Breakdown Spectroscopy (LIBS) for Application to MSL Chemc
    Journal of Geophysical Research: Planets RESEARCH ARTICLE Characterization of Hydrogen in Basaltic Materials With 10.1029/2017JE005467 Laser-Induced Breakdown Spectroscopy (LIBS) Key Points: for Application to MSL ChemCam Data • Multiple calibration and normalization methods to determine N. H. Thomas1 , B. L. Ehlmann1,2 , D. E. Anderson1 , S. M. Clegg3 , O. Forni4 , S. Schröder4,5, hydrogen content from the 1 4 4 3 6 4 hydrogen-alpha LIBS emission line W. Rapin , P.-Y. Meslin , J. Lasue , D. M. Delapp , M. D. Dyar , O. Gasnault , 3 4 were evaluated R. C. Wiens , and S. Maurice • O 778- and C 248-nm norms have the lowest scatter for the lab set, best 1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA, 2Jet Propulsion correct for distance, and successfully Laboratory, California Institute of Technology, Pasadena, CA, USA, 3Los Alamos National Laboratory, Los Alamos, NM, USA, determine H for Martian rocks 4 5 • Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, Toulouse, France, German Aerospace Nonlinear calibrations for high-H 6 samples and differences in H Center (DLR), Berlin, Germany, Mount Holyoke College, South Hadley, MA, USA between rocks, when natural versus pelletized, warrant further study Abstract The Mars Science Laboratory rover, Curiosity, is equipped with ChemCam, a laser-induced breakdown spectroscopy (LIBS) instrument, to determine the elemental composition of nearby targets Supporting Information: • Supporting Information S1 quickly and remotely. We use a laboratory sample set including prepared mixtures of basalt with systematic • Data Set S1 variation in hydrated mineral content and compositionally well-characterized, altered basaltic volcanic rocks to measure hydrogen by characterizing the H-alpha emission line in LIBS spectra under Martian Correspondence to: environmental conditions.
    [Show full text]
  • FY 2009 Geosciences Research
    Summary of FY 2009 Geosciences Research August 2010 U.S. Department of Energy Office of Science Office of Basic Energy Sciences Chemical Sciences, Geosciences, and Biosciences Division Washington, D.C. 20585 TABLE OF CONTENTS TABLE OF CONTENTS .........................................................................................................................2 FORWARD .............................................................................................................................................10 THE GEOSCIENCES RESEARCH PROGRAM IN THE OFFICE OF BASIC ENERGY SCIENCES..........................................................................................................................................11 ARGONNE NATIONAL LABORATORY .........................................................................................12 Mineral-Fluid Interactions: Synchrotron Radiation Studies at the Advanced Photon Source .................12 IDAHO NATIONAL LABORATORY ................................................................................................14 Pathways for Redox Transformation of Semiconducting Minerals: The Iron Oxides .............................14 LAWRENCE BERKELEY NATIONAL LABORATORY ...............................................................16 Upgrade of the Computational Cluster at LBNL .....................................................................................16 Center for Nanoscale Control of Geologic CO2 .......................................................................................16
    [Show full text]
  • Properties of Deep Weathered Swelling Clay and Its Stability Implications in Tunneling
    TGB4930 Engineering Geology and Rock Mechanics Master’s Thesis Leena Jaakola Properties of Deep Weathered Swelling Clay and its Stability Implications in Tunneling Trondheim, 10 June, 2019 NTNU Norwegian University of Science and Technology Faculty of Engineering Department of Geoscience and Petroleum Abstract Remains of subtropical deep weathered clay found in fracture and weakness zones in the bedrock in the Trøndelag area yields poor conditions for tunnel construction and have re- sulted in expensive difficulties for such projects. Smectite has a high swelling potential when hydrated, which can induce swelling pressure and damage the structures it surrounds. This study was designed as an extension of a previous study performed at NTNU that showed ambiguity between free swell and swelling pressure measurements. 55 samples exhibiting swelling behavior were obtained from old SINTEF projects. Swelling minerals were identi- fied using X-Ray diffraction and the fine particle fraction grain size distribution was measured using laser diffraction spectroscopy. Swelling potential was quantified using constant volume oedometer testing and free swell tests. The potential of variance (r2) between mineral con- tent and maximum swelling pressure was 0.8. Free swell was less correlated with smectite content, yielding an r2 value of 0.4 and several outliers. Free swell was affected by other physical parameters in addition to smectite content. Additional tests, which could not be performed due to limited sample material, are desired to better understand the physical properties behind each measure of swelling potential. i CONTENTS Contents 1 Introduction 1 1.1 Purpose and Objectives of this Study . .1 1.2 Background . .1 1.3 Swelling Potential .
    [Show full text]
  • Clay Neomineralization and the Timing, Thermal Conditions and Geofluid History of Upper Crustal Deformation Zones
    Clay Neomineralization and the Timing, Thermal Conditions and Geofluid History of Upper Crustal Deformation Zones by Austin Harold Boles A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (Earth and Environmental Sciences) in The University of Michigan 2017 Doctoral Committee: Professor Ben van der Pluijm, Chair Professor Jeffrey C. Alt Professor Richard B. Rood Emeritus Professor Rob Van Der Voo Corrigendum 4/20/2018 After publication of this dissertation, an equipment malfunction was discovered that affects the dataset included in Chapter VI, “Triassic, Surface-Fluid Derived Clay Diagenesis in the Appalachian Plateau, Northern U.S. Midcontinent.” Reanalysis and corrections are currently being applied, but until that dataset has been published in peer-reviewed literature, the 40Ar/39Ar geochronology reported herein and its interpretation SHOULD NOT BE USED, either for citation or as a basis for further research. The dissertation committee of Austin Boles, listed below, approves this corrigendum and its insertion into the dissertation: Ben van der Pluijm, Chair Richard B. Rood Jeffrey Alt Rob Van Der Voo Satur venter non studet libenter A view of the Southern Alpine Orogen, South Island, New Zealand. Field photo (2014). Austin Harold Boles [email protected]; [email protected] ORCID iD: 0000-0003-3072-3309 Copyright © Austin Harold Boles 2017 All Rights Reserved Dedication I dedicate this volume to my two sons, Oliver and Calum. May they be ever curious and never lose their wonder. ii Acknowledgments I thank the many collaborators, colleagues, mentors, committee members and friends who have supported, encouraged, and taught me along the way: Anja Schleicher, Eliza Fitz-Diaz, Samantha Nemkin, Erin Lynch, Brice Lacroix, Jasmaria Wojtschke, Bernhard Schuck, Semih Can Ülgen, Celal Şengör, Halim Mutlu, I.
    [Show full text]
  • Download This Article in PDF Format
    E3S Web of Conferences 244, 04008 (2021) https://doi.org/10.1051/e3sconf/202124404008 EMMFT-2020 Morphology of ettringite crystal of sulfoferrite clinker Dmitriy Zorin1,* and Ivan Burlov2 1The Moscow State University of Civil Engineering (National Rresearch University), Yaroslavskoye shosse, 26, 125993, Moscow, Russia 2Mendeleev University of Chemical Technology, Miusskaya square, 9, 125047, Moscow, Russia Abstract. This paper deals with the composition and properties of solid solution of calcium sulfoferrite. It was studied an influence of calcium s sulfoferrite on structure and properties cement phases. Study of the hydration processes of the calcium sulfoferrite mineral are observed only short prismatic crystals. Prismatic crystals of ferruginous ettringite are always formed from sulfoferrite mineral of any fraction. it was found that the smaller the initial hydrating grains of minerals, the faster they are hydrated. Analyse polyfractional compound hydration showed that fine fractions provide formation of crystallization centres, and particles less than 45 microns, with constant interaction with the liquid phase, cause a gradual growth of crystals. Expansion of hydrated minerals of certain fractions was analysed to check the dependence of the expansion on the morphology of ettringite crystal hydrates. During the hardening of the samples, expansion was observed along with a drop in strength. 1 Introduction Hydration and hardening of Portland cement are accompanied by generating of crystalline and gel-like products, which, together with non-hydrated grains, participate in formation of the three-dimensional framework of the cement stone[1-3]. Depending on activity of the original mineral, the crystalline hydrates are formed sequentially or simultaneously, while they filling the free space in the cement stone.
    [Show full text]
  • DIFFUSE REFLECTANCE SPECTRA of Sevtrral CLAY MINERALS
    American Mineralogist Vol. 57, pp. 485-493 (1972) DIFFUSEREFLECTANCE SPECTRA OF SEVtrRAL CLAY MINERALS Jerrns D. LrNnsERc AND DAVID G. SNvnnn, Atm,ospheri'c Sciences Labor'atory, US Armg Electr'onics Contmand, White Sunds Missile Ram,ge,New Meriao 88002 Assrnecr The diffuse reflectance spectra in the 0.3 to 2.1 micrometer wavelength region have been measured for several sa,mples of clay minerals sometimes found in the atmospheric aerosol. Exa.mples of spectra are shown for different hydration states of several montmorillonite and kaolin group minerals. It was found that these clays show absorption features in the wavelength regions where liquid water absorbs. These absorption bands are removed by dehydration, as would be expected.It is concludedthat the major features of the near infrared absorp- tion spectra of montmorillonite and kaolin clays are determined primarily by the water present in the clay stmctures. In addition, the spectra show evidence of strong absorption in the near ultraviolet and short wavelength visible region. This latter absorption is a general feature of all the clay samples investigated. INrnooucrroN In connection with this laboratory's interest in the properties of atmospheric dust it has becornenecessary to obtain some information about,the absorption spectra of several clay minerals in the near ultra- violet, visible, and near infrared spectral regions. Previous work (Hoidale and Blanco, 1969) has shown that the clay minerals mont- morillonite, kaolinite, and illite are likely to be significant constituents of atmospheric dust, at least in arid desert regions. The spectra for most clay minerals have been determined by several workersl for wa,velengths longer than about two micrometers, using alkali halide disk or liquid mull infrared spectroscopic techniques.
    [Show full text]
  • Molecular Dynamics Simulation of Clay Hydration Inhibition of Deep Shale
    processes Article Molecular Dynamics Simulation of Clay Hydration Inhibition of Deep Shale Yayun Zhang 1,2 and Cong Xiao 3,* 1 State Key Laboratory of Shale Oil and Gas Enrichment Mechanisms and Effective Development, Beijing 100101, China; [email protected] 2 Sinopec Research Institute of Petroleum Engineering, Beijing 100101, China 3 Delft Institute of Applied Mathematics, Delft University of Technology, Mekelweg 4, 2628 CD Delft, The Netherlands * Correspondence: [email protected] Abstract: In the process of the exploitation of deep oil and gas resources, shale wellbore stability control faces great challenges under complex temperature and pressure conditions. It is difficult to reflect the micro mechanism and process of the action of inorganic salt on shale hydration with the traditional experimental evaluation technology on the macro effect of restraining shale hydra- tion. Aiming at the characteristics of clay minerals of deep shale, the molecular dynamics models + + + 2+ of four typical cations (K , NH4 , Cs and Ca ) inhibiting the hydration of clay minerals have been established by the use of the molecular dynamics simulation method. Moreover, the micro dynamics mechanism of typical inorganic cations inhibiting the hydration of clay minerals has been systematically evaluated, as has the law of cation hydration inhibition performance in response to temperature, pressure and ion type. The research indicates that the cations can promote the contraction of interlayer spacing, compress fluid intrusion channels, reduce the intrusion ability of water molecules, increase the negative charge balance ability and reduce the interlayer electrostatic repulsion force. With the increase in temperature, the inhibition of the cations on montmorillonite Citation: Zhang, Y.; Xiao, C.
    [Show full text]
  • Curiosity Mars Rover Sees Trend in Water Presence 18 March 2013
    Curiosity Mars rover sees trend in water presence 18 March 2013 into the ground to probe for hydrogen, researchers have found more hydration of minerals near the clay-bearing rock than at locations Curiosity visited earlier. The rover's Mast Camera (Mastcam) can also serve as a mineral-detecting and hydration- detecting tool, reported Jim Bell of Arizona State University, Tempe. "Some iron-bearing rocks and minerals can be detected and mapped using the Mastcam's near-infrared filters." On this image of the rock target "Knorr," color coding maps the amount of mineral hydration indicated by a ratio of near-infrared reflectance intensities measured by the Mast Camera (Mastcam) on NASA's Mars rover Curiosity. Credit: NASA/JPL-Caltech/MSSS/ASU (Phys.org) —NASA's Mars rover Curiosity has seen evidence of water-bearing minerals in rocks near where it had already found clay minerals inside a The gray area in the center of this image is where the drilled rock. Dust Removal Tool on the robotic arm of NASA's Mars rover Curiosity brushed a rock target called "Wernecke." Last week, the rover's science team announced The brushing revealed dark nodules and white veins that analysis of powder from a drilled mudstone crisscrossing the light gray rock. The brushed area is about 2.5 inches (6 centimeters) across. The Mars Hand rock on Mars indicates past environmental Lens Imager (MAHLI) camera on the rover's arm took this conditions that were favorable for microbial life. image during the 169th Martian day, or sol, of Curiosity's Additional findings presented today (March 18) at a mission on Mars (Jan.
    [Show full text]